Similar Matrices and Jordan Form

Total Page:16

File Type:pdf, Size:1020Kb

Similar Matrices and Jordan Form Similar matrices and Jordan form We’ve nearly covered the entire heart of linear algebra – once we’ve finished singular value decompositions we’ll have seen all the most central topics. AT A is positive definite A matrix is positive definite if xT Ax > 0 for all x 6= 0. This is a very important class of matrices; positive definite matrices appear in the form of AT A when computing least squares solutions. In many situations, a rectangular matrix is multiplied by its transpose to get a square matrix. Given a symmetric positive definite matrix A, is its inverse also symmet­ ric and positive definite? Yes, because if the (positive) eigenvalues of A are −1 l1, l2, · · · ld then the eigenvalues 1/l1, 1/l2, · · · 1/ld of A are also positive. If A and B are positive definite, is A + B positive definite? We don’t know much about the eigenvalues of A + B, but we can use the property xT Ax > 0 and xT Bx > 0 to show that xT(A + B)x > 0 for x 6= 0 and so A + B is also positive definite. Now suppose A is a rectangular (m by n) matrix. A is almost certainly not symmetric, but AT A is square and symmetric. Is AT A positive definite? We’d rather not try to find the eigenvalues or the pivots of this matrix, so we ask when xT AT Ax is positive. Simplifying xT AT Ax is just a matter of moving parentheses: xT (AT A)x = (Ax)T (Ax) = jAxj2 ≥ 0. The only remaining question is whether Ax = 0. If A has rank n (independent columns), then xT (AT A)x = 0 only if x = 0 and A is positive definite. Another nice feature of positive definite matrices is that you never have to do row exchanges when row reducing – there are never 0’s or unsuitably small numbers in their pivot positions. Similar matrices A and B = M−1 AM Two square matrices A and B are similar if B = M−1 AM for some matrix M. This allows us to put matrices into families in which all the matrices in a family are similar to each other. Then each family can be represented by a diagonal (or nearly diagonal) matrix. Distinct eigenvalues If A has a full set of eigenvectors we can create its eigenvector matrix S and write S−1 AS = L. So A is similar to L (choosing M to be this S). 1 � � � � � � 2 1 3 0 3 0 If A = then L = and so A is similar to . But A 1 2 0 1 0 1 is also similar to: −1 M A M B � 1 −4 � � 3 0 � � 1 4 � � 1 −4 � � 2 9 � = 0 1 0 1 0 1 0 1 1 6 � −2 −15 � = . 1 6 In addition, B is similar to L. All these similar matrices have the same eigen­ values, 3 and 1; we can check this by computing the trace and determinant of A and B. Similar matrices have the same eigenvalues! In fact, the matrices similar to A are all the 2 by 2 matrices with eigenvalues � � � � 3 7 1 7 3 and 1. Some other members of this family are and . To 0 1 0 3 prove that similar matrices have the same eigenvalues, suppose Ax = lx. We modify this equation to include B = M−1 AM: AMM−1x = lx M−1 AMM−1x = lM−1x BM−1x = lM−1x. The matrix B has the same l as an eigenvalue. M−1x is the eigenvector. If two matrices are similar, they have the same eigenvalues and the same number of independent eigenvectors (but probably not the same eigenvectors). When we diagonalize A, we’re finding a diagonal matrix L that is similar to A. If two matrices have the same n distinct eigenvalues, they’ll be similar to the same diagonal matrix. Repeated eigenvalues If two eigenvalues of A are the same, it may not be possible to diagonalize A. Suppose l1 = l2 = 4. One family of matrices with eigenvalues 4 and 4 � � � � 4 0 4 1 contains only the matrix . The matrix is not in this family. 0 4 0 4 There are two families of similar matrices with eigenvalues 4 and 4. The � � 4 1 larger family includes . Each of the members of this family has only 0 4 one eigenvector. � � 4 0 The matrix is the only member of the other family, because: 0 4 � 4 0 � � 4 0 � M−1 M = 4M−1 M = 0 4 0 4 for any invertible matrix M. 2 Jordan form Camille Jordan found a way to choose a “most diagonal” representative from each family of similar matrices; this representative is said to be in Jordan nor­ � � � � 4 1 4 0 mal form. For example, both and are in Jordan form. This 0 4 0 4 form used to be the climax of linear algebra, but not any more. Numerical applications rarely need it. � � 4 1 We can find more members of the family represented by by choos­ 0 4 ing diagonal entries to get a trace of 4, then choosing off-diagonal entries to get a determinant of 16: � 4 1 � � 5 1 � � 4 0 � � a b � , , , . 0 4 −1 3 17 4 (8a − a2 − 16)/b 8 − a (None of these are diagonalizable, because if they were they would be similar � � 4 0 to . That matrix is only similar to itself.) What about this one? 0 4 2 0 1 0 0 3 6 0 0 1 0 7 A = 6 7 4 0 0 0 0 5 0 0 0 0 Its eigenvalues are four zeros. Its rank is 2 so the dimension of its nullspace is 4 − 2 = 2. It will have two independent eigenvectors and two “missing” eigenvectors. When we look instead at 2 0 1 7 0 3 6 0 0 1 0 7 6 7 , 4 0 0 0 0 5 0 0 0 0 its rank and the dimension of its nullspace are still 2, but it’s not as nice as A. B is similar to A, which is the Jordan normal form representative of this family. A has a 1 above the diagonal for every missing eigenvector and the rest of its entries are 0. Now consider: 2 0 1 0 0 3 6 0 0 0 0 7 C = 6 7 . 4 0 0 0 1 5 0 0 0 0 Again it has rank 2 and its nullspace has dimension 2. Its four eigenvalues are 0. Surprisingly, it is not similar to A. We can see this by breaking the matrices 3 into their Jordan blocks: 2 0 1 0 0 3 2 0 1 0 0 3 6 0 0 1 0 7 6 0 0 0 0 7 A = 6 7 , C = 6 7 . 4 0 0 0 0 5 4 0 0 0 1 5 0 0 0 0 0 0 0 0 A Jordan block Ji has a repeated eigenvalue li on the diagonal, zeros below the diagonal and in the upper right hand corner, and ones above the diagonal: 2 3 li 1 0 · · · 0 6 0 li 1 0 7 6 7 6 . 7 Ji = 6 . .. 7 . 6 7 4 0 0 li 1 5 0 0 · · · 0 li Two matrices may have the same eigenvalues and the same number of eigen­ vectors, but if their Jordan blocks are different sizes those matrices can not be similar. Jordan’s theorem says that every square matrix A is similar to a Jordan matrix J, with Jordan blocks on the diagonal: 2 3 J1 0 · · · 0 6 0 J2 · · · 0 7 6 7 J = 6 . 7 . 4 . .. 5 0 0 · · · Jd In a Jordan matrix, the eigenvalues are on the diagonal and there may be ones above the diagonal; the rest of the entries are zero. The number of blocks is the number of eigenvectors – there is one eigenvector per block. To summarize: • If A has n distinct eigenvalues, it is diagonalizable and its Jordan matrix is the diagonal matrix J = L. • If A has repeated eigenvalues and “missing” eigenvectors, then its Jordan matrix will have n − d ones above the diagonal. We have not learned to compute the Jordan matrix of a matrix which is missing eigenvectors, but we do know how to diagonalize a matrix which has n distinct eigenvalues. 4 MIT OpenCourseWare http://ocw.mit.edu 18.06SC Linear Algebra Fall 2011 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. .
Recommended publications
  • Regular Linear Systems on Cp1 and Their Monodromy Groups V.P
    Astérisque V. P. KOSTOV Regular linear systems onCP1 and their monodromy groups Astérisque, tome 222 (1994), p. 259-283 <http://www.numdam.org/item?id=AST_1994__222__259_0> © Société mathématique de France, 1994, tous droits réservés. L’accès aux archives de la collection « Astérisque » (http://smf4.emath.fr/ Publications/Asterisque/) implique l’accord avec les conditions générales d’uti- lisation (http://www.numdam.org/conditions). Toute utilisation commerciale ou impression systématique est constitutive d’une infraction pénale. Toute copie ou impression de ce fichier doit contenir la présente mention de copyright. Article numérisé dans le cadre du programme Numérisation de documents anciens mathématiques http://www.numdam.org/ REGULAR LINEAR SYSTEMS ON CP1 AND THEIR MONODROMY GROUPS V.P. KOSTOV 1. INTRODUCTION 1.1 A meromorphic linear system of differential equations on CP1 can be pre­ sented in the form X = A(t)X (1) where A{t) is a meromorphic on CP1 n x n matrix function, " • " = d/dt. Denote its poles ai,... ,ap+i, p > 1. We consider the dependent variable X to be also n x n-matrix. Definition. System (1) is called fuchsian if all the poles of the matrix- function A(t) axe of first order. Definition. System (1) is called regular at the pole a,j if in its neighbour­ hood the solutions of the system are of moderate growth rate, i.e. IW-a^l^Odt-a^), Ni E R, j = 1,...., p + 1 Here || • || denotes an arbitrary norm in gl(n, C) and we consider a restriction of the solution to a sector with vertex at ctj and of a sufficiently small radius, i.e.
    [Show full text]
  • The Rational and Jordan Forms Linear Algebra Notes
    The Rational and Jordan Forms Linear Algebra Notes Satya Mandal November 5, 2005 1 Cyclic Subspaces In a given context, a "cyclic thing" is an one generated "thing". For example, a cyclic groups is a one generated group. Likewise, a module M over a ring R is said to be a cyclic module if M is one generated or M = Rm for some m 2 M: We do not use the expression "cyclic vector spaces" because one generated vector spaces are zero or one dimensional vector spaces. 1.1 (De¯nition and Facts) Suppose V is a vector space over a ¯eld F; with ¯nite dim V = n: Fix a linear operator T 2 L(V; V ): 1. Write R = F[T ] = ff(T ) : f(X) 2 F[X]g L(V; V )g: Then R = F[T ]g is a commutative ring. (We did considered this ring in last chapter in the proof of Caley-Hamilton Theorem.) 2. Now V acquires R¡module structure with scalar multiplication as fol- lows: Define f(T )v = f(T )(v) 2 V 8 f(T ) 2 F[T ]; v 2 V: 3. For an element v 2 V de¯ne Z(v; T ) = F[T ]v = ff(T )v : f(T ) 2 Rg: 1 Note that Z(v; T ) is the cyclic R¡submodule generated by v: (I like the notation F[T ]v, the textbook uses the notation Z(v; T ).) We say, Z(v; T ) is the T ¡cyclic subspace generated by v: 4. If V = Z(v; T ) = F[T ]v; we say that that V is a T ¡cyclic space, and v is called the T ¡cyclic generator of V: (Here, I di®er a little from the textbook.) 5.
    [Show full text]
  • MAT247 Algebra II Assignment 5 Solutions
    MAT247 Algebra II Assignment 5 Solutions 1. Find the Jordan canonical form and a Jordan basis for the map or matrix given in each part below. (a) Let V be the real vector space spanned by the polynomials xiyj (in two variables) with i + j ≤ 3. Let T : V V be the map Dx + Dy, where Dx and Dy respectively denote 2 differentiation with respect to x and y. (Thus, Dx(xy) = y and Dy(xy ) = 2xy.) 0 1 1 1 1 1 ! B0 1 2 1 C (b) A = B C over Q @0 0 1 -1A 0 0 0 2 Solution: (a) The operator T is nilpotent so its characterictic polynomial splits and its only eigenvalue is zero and K0 = V. We have Im(T) = spanf1; x; y; x2; xy; y2g; Im(T 2) = spanf1; x; yg Im(T 3) = spanf1g T 4 = 0: Thus the longest cycle for eigenvalue zero has length 4. Moreover, since the number of cycles of length at least r is given by dim(Im(T r-1)) - dim(Im(T r)), the number of cycles of lengths at least 4, 3, 2, 1 is respectively 1, 2, 3, and 4. Thus the number of cycles of lengths 4,3,2,1 is respectively 1,1,1,1. Denoting the r × r Jordan block with λ on the diagonal by Jλ,r, the Jordan canonical form is thus 0 1 J0;4 B J0;3 C J = B C : @ J0;2 A J0;1 We now proceed to find a corresponding Jordan basis, i.e.
    [Show full text]
  • Estimations of the Trace of Powers of Positive Self-Adjoint Operators by Extrapolation of the Moments∗
    Electronic Transactions on Numerical Analysis. ETNA Volume 39, pp. 144-155, 2012. Kent State University Copyright 2012, Kent State University. http://etna.math.kent.edu ISSN 1068-9613. ESTIMATIONS OF THE TRACE OF POWERS OF POSITIVE SELF-ADJOINT OPERATORS BY EXTRAPOLATION OF THE MOMENTS∗ CLAUDE BREZINSKI†, PARASKEVI FIKA‡, AND MARILENA MITROULI‡ Abstract. Let A be a positive self-adjoint linear operator on a real separable Hilbert space H. Our aim is to build estimates of the trace of Aq, for q ∈ R. These estimates are obtained by extrapolation of the moments of A. Applications of the matrix case are discussed, and numerical results are given. Key words. Trace, positive self-adjoint linear operator, symmetric matrix, matrix powers, matrix moments, extrapolation. AMS subject classifications. 65F15, 65F30, 65B05, 65C05, 65J10, 15A18, 15A45. 1. Introduction. Let A be a positive self-adjoint linear operator from H to H, where H is a real separable Hilbert space with inner product denoted by (·, ·). Our aim is to build estimates of the trace of Aq, for q ∈ R. These estimates are obtained by extrapolation of the integer moments (z, Anz) of A, for n ∈ N. A similar procedure was first introduced in [3] for estimating the Euclidean norm of the error when solving a system of linear equations, which corresponds to q = −2. The case q = −1, which leads to estimates of the trace of the inverse of a matrix, was studied in [4]; on this problem, see [10]. Let us mention that, when only positive powers of A are used, the Hilbert space H could be infinite dimensional, while, for negative powers of A, it is always assumed to be a finite dimensional one, and, obviously, A is also assumed to be invertible.
    [Show full text]
  • The Invertible Matrix Theorem
    The Invertible Matrix Theorem Ryan C. Daileda Trinity University Linear Algebra Daileda The Invertible Matrix Theorem Introduction It is important to recognize when a square matrix is invertible. We can now characterize invertibility in terms of every one of the concepts we have now encountered. We will continue to develop criteria for invertibility, adding them to our list as we go. The invertibility of a matrix is also related to the invertibility of linear transformations, which we discuss below. Daileda The Invertible Matrix Theorem Theorem 1 (The Invertible Matrix Theorem) For a square (n × n) matrix A, TFAE: a. A is invertible. b. A has a pivot in each row/column. RREF c. A −−−→ I. d. The equation Ax = 0 only has the solution x = 0. e. The columns of A are linearly independent. f. Null A = {0}. g. A has a left inverse (BA = In for some B). h. The transformation x 7→ Ax is one to one. i. The equation Ax = b has a (unique) solution for any b. j. Col A = Rn. k. A has a right inverse (AC = In for some C). l. The transformation x 7→ Ax is onto. m. AT is invertible. Daileda The Invertible Matrix Theorem Inverse Transforms Definition A linear transformation T : Rn → Rn (also called an endomorphism of Rn) is called invertible iff it is both one-to-one and onto. If [T ] is the standard matrix for T , then we know T is given by x 7→ [T ]x. The Invertible Matrix Theorem tells us that this transformation is invertible iff [T ] is invertible.
    [Show full text]
  • 5 the Dirac Equation and Spinors
    5 The Dirac Equation and Spinors In this section we develop the appropriate wavefunctions for fundamental fermions and bosons. 5.1 Notation Review The three dimension differential operator is : ∂ ∂ ∂ = , , (5.1) ∂x ∂y ∂z We can generalise this to four dimensions ∂µ: 1 ∂ ∂ ∂ ∂ ∂ = , , , (5.2) µ c ∂t ∂x ∂y ∂z 5.2 The Schr¨odinger Equation First consider a classical non-relativistic particle of mass m in a potential U. The energy-momentum relationship is: p2 E = + U (5.3) 2m we can substitute the differential operators: ∂ Eˆ i pˆ i (5.4) → ∂t →− to obtain the non-relativistic Schr¨odinger Equation (with = 1): ∂ψ 1 i = 2 + U ψ (5.5) ∂t −2m For U = 0, the free particle solutions are: iEt ψ(x, t) e− ψ(x) (5.6) ∝ and the probability density ρ and current j are given by: 2 i ρ = ψ(x) j = ψ∗ ψ ψ ψ∗ (5.7) | | −2m − with conservation of probability giving the continuity equation: ∂ρ + j =0, (5.8) ∂t · Or in Covariant notation: µ µ ∂µj = 0 with j =(ρ,j) (5.9) The Schr¨odinger equation is 1st order in ∂/∂t but second order in ∂/∂x. However, as we are going to be dealing with relativistic particles, space and time should be treated equally. 25 5.3 The Klein-Gordon Equation For a relativistic particle the energy-momentum relationship is: p p = p pµ = E2 p 2 = m2 (5.10) · µ − | | Substituting the equation (5.4), leads to the relativistic Klein-Gordon equation: ∂2 + 2 ψ = m2ψ (5.11) −∂t2 The free particle solutions are plane waves: ip x i(Et p x) ψ e− · = e− − · (5.12) ∝ The Klein-Gordon equation successfully describes spin 0 particles in relativistic quan- tum field theory.
    [Show full text]
  • QUADRATIC FORMS and DEFINITE MATRICES 1.1. Definition of A
    QUADRATIC FORMS AND DEFINITE MATRICES 1. DEFINITION AND CLASSIFICATION OF QUADRATIC FORMS 1.1. Definition of a quadratic form. Let A denote an n x n symmetric matrix with real entries and let x denote an n x 1 column vector. Then Q = x’Ax is said to be a quadratic form. Note that a11 ··· a1n . x1 Q = x´Ax =(x1...xn) . xn an1 ··· ann P a1ixi . =(x1,x2, ··· ,xn) . P anixi 2 (1) = a11x1 + a12x1x2 + ... + a1nx1xn 2 + a21x2x1 + a22x2 + ... + a2nx2xn + ... + ... + ... 2 + an1xnx1 + an2xnx2 + ... + annxn = Pi ≤ j aij xi xj For example, consider the matrix 12 A = 21 and the vector x. Q is given by 0 12x1 Q = x Ax =[x1 x2] 21 x2 x1 =[x1 +2x2 2 x1 + x2 ] x2 2 2 = x1 +2x1 x2 +2x1 x2 + x2 2 2 = x1 +4x1 x2 + x2 1.2. Classification of the quadratic form Q = x0Ax: A quadratic form is said to be: a: negative definite: Q<0 when x =06 b: negative semidefinite: Q ≤ 0 for all x and Q =0for some x =06 c: positive definite: Q>0 when x =06 d: positive semidefinite: Q ≥ 0 for all x and Q = 0 for some x =06 e: indefinite: Q>0 for some x and Q<0 for some other x Date: September 14, 2004. 1 2 QUADRATIC FORMS AND DEFINITE MATRICES Consider as an example the 3x3 diagonal matrix D below and a general 3 element vector x. 100 D = 020 004 The general quadratic form is given by 100 x1 0 Q = x Ax =[x1 x2 x3] 020 x2 004 x3 x1 =[x 2 x 4 x ] x2 1 2 3 x3 2 2 2 = x1 +2x2 +4x3 Note that for any real vector x =06 , that Q will be positive, because the square of any number is positive, the coefficients of the squared terms are positive and the sum of positive numbers is always positive.
    [Show full text]
  • A Some Basic Rules of Tensor Calculus
    A Some Basic Rules of Tensor Calculus The tensor calculus is a powerful tool for the description of the fundamentals in con- tinuum mechanics and the derivation of the governing equations for applied prob- lems. In general, there are two possibilities for the representation of the tensors and the tensorial equations: – the direct (symbolic) notation and – the index (component) notation The direct notation operates with scalars, vectors and tensors as physical objects defined in the three dimensional space. A vector (first rank tensor) a is considered as a directed line segment rather than a triple of numbers (coordinates). A second rank tensor A is any finite sum of ordered vector pairs A = a b + ... +c d. The scalars, vectors and tensors are handled as invariant (independent⊗ from the choice⊗ of the coordinate system) objects. This is the reason for the use of the direct notation in the modern literature of mechanics and rheology, e.g. [29, 32, 49, 123, 131, 199, 246, 313, 334] among others. The index notation deals with components or coordinates of vectors and tensors. For a selected basis, e.g. gi, i = 1, 2, 3 one can write a = aig , A = aibj + ... + cidj g g i i ⊗ j Here the Einstein’s summation convention is used: in one expression the twice re- peated indices are summed up from 1 to 3, e.g. 3 3 k k ik ik a gk ∑ a gk, A bk ∑ A bk ≡ k=1 ≡ k=1 In the above examples k is a so-called dummy index. Within the index notation the basic operations with tensors are defined with respect to their coordinates, e.
    [Show full text]
  • Math 54. Selected Solutions for Week 8 Section 6.1 (Page 282) 22. Let U = U1 U2 U3 . Explain Why U · U ≥ 0. Wh
    Math 54. Selected Solutions for Week 8 Section 6.1 (Page 282) 2 3 u1 22. Let ~u = 4 u2 5 . Explain why ~u · ~u ≥ 0 . When is ~u · ~u = 0 ? u3 2 2 2 We have ~u · ~u = u1 + u2 + u3 , which is ≥ 0 because it is a sum of squares (all of which are ≥ 0 ). It is zero if and only if ~u = ~0 . Indeed, if ~u = ~0 then ~u · ~u = 0 , as 2 can be seen directly from the formula. Conversely, if ~u · ~u = 0 then all the terms ui must be zero, so each ui must be zero. This implies ~u = ~0 . 2 5 3 26. Let ~u = 4 −6 5 , and let W be the set of all ~x in R3 such that ~u · ~x = 0 . What 7 theorem in Chapter 4 can be used to show that W is a subspace of R3 ? Describe W in geometric language. The condition ~u · ~x = 0 is equivalent to ~x 2 Nul ~uT , and this is a subspace of R3 by Theorem 2 on page 187. Geometrically, it is the plane perpendicular to ~u and passing through the origin. 30. Let W be a subspace of Rn , and let W ? be the set of all vectors orthogonal to W . Show that W ? is a subspace of Rn using the following steps. (a). Take ~z 2 W ? , and let ~u represent any element of W . Then ~z · ~u = 0 . Take any scalar c and show that c~z is orthogonal to ~u . (Since ~u was an arbitrary element of W , this will show that c~z is in W ? .) ? (b).
    [Show full text]
  • Jordan Decomposition for Differential Operators Samuel Weatherhog Bsc Hons I, BE Hons IIA
    Jordan Decomposition for Differential Operators Samuel Weatherhog BSc Hons I, BE Hons IIA A thesis submitted for the degree of Master of Philosophy at The University of Queensland in 2017 School of Mathematics and Physics i Abstract One of the most well-known theorems of linear algebra states that every linear operator on a complex vector space has a Jordan decomposition. There are now numerous ways to prove this theorem, how- ever a standard method of proof relies on the existence of an eigenvector. Given a finite-dimensional, complex vector space V , every linear operator T : V ! V has an eigenvector (i.e. a v 2 V such that (T − λI)v = 0 for some λ 2 C). If we are lucky, V may have a basis consisting of eigenvectors of T , in which case, T is diagonalisable. Unfortunately this is not always the case. However, by relaxing the condition (T − λI)v = 0 to the weaker condition (T − λI)nv = 0 for some n 2 N, we can always obtain a basis of generalised eigenvectors. In fact, there is a canonical decomposition of V into generalised eigenspaces and this is essentially the Jordan decomposition. The topic of this thesis is an analogous theorem for differential operators. The existence of a Jordan decomposition in this setting was first proved by Turrittin following work of Hukuhara in the one- dimensional case. Subsequently, Levelt proved uniqueness and provided a more conceptual proof of the original result. As a corollary, Levelt showed that every differential operator has an eigenvector. He also noted that this was a strange chain of logic: in the linear setting, the existence of an eigen- vector is a much easier result and is in fact used to obtain the Jordan decomposition.
    [Show full text]
  • 18.700 JORDAN NORMAL FORM NOTES These Are Some Supplementary Notes on How to Find the Jordan Normal Form of a Small Matrix. Firs
    18.700 JORDAN NORMAL FORM NOTES These are some supplementary notes on how to find the Jordan normal form of a small matrix. First we recall some of the facts from lecture, next we give the general algorithm for finding the Jordan normal form of a linear operator, and then we will see how this works for small matrices. 1. Facts Throughout we will work over the field C of complex numbers, but if you like you may replace this with any other algebraically closed field. Suppose that V is a C-vector space of dimension n and suppose that T : V → V is a C-linear operator. Then the characteristic polynomial of T factors into a product of linear terms, and the irreducible factorization has the form m1 m2 mr cT (X) = (X − λ1) (X − λ2) ... (X − λr) , (1) for some distinct numbers λ1, . , λr ∈ C and with each mi an integer m1 ≥ 1 such that m1 + ··· + mr = n. Recall that for each eigenvalue λi, the eigenspace Eλi is the kernel of T − λiIV . We generalized this by defining for each integer k = 1, 2,... the vector subspace k k E(X−λi) = ker(T − λiIV ) . (2) It is clear that we have inclusions 2 e Eλi = EX−λi ⊂ E(X−λi) ⊂ · · · ⊂ E(X−λi) ⊂ .... (3) k k+1 Since dim(V ) = n, it cannot happen that each dim(E(X−λi) ) < dim(E(X−λi) ), for each e e +1 k = 1, . , n. Therefore there is some least integer ei ≤ n such that E(X−λi) i = E(X−λi) i .
    [Show full text]
  • (VI.E) Jordan Normal Form
    (VI.E) Jordan Normal Form Set V = Cn and let T : V ! V be any linear transformation, with distinct eigenvalues s1,..., sm. In the last lecture we showed that V decomposes into stable eigenspaces for T : s s V = W1 ⊕ · · · ⊕ Wm = ker (T − s1I) ⊕ · · · ⊕ ker (T − smI). Let B = fB1,..., Bmg be a basis for V subordinate to this direct sum and set B = [T j ] , so that k Wk Bk [T]B = diagfB1,..., Bmg. Each Bk has only sk as eigenvalue. In the event that A = [T]eˆ is s diagonalizable, or equivalently ker (T − skI) = ker(T − skI) for all k , B is an eigenbasis and [T]B is a diagonal matrix diagf s1,..., s1 ;...; sm,..., sm g. | {z } | {z } d1=dim W1 dm=dim Wm Otherwise we must perform further surgery on the Bk ’s separately, in order to transform the blocks Bk (and so the entire matrix for T ) into the “simplest possible” form. The attentive reader will have noticed above that I have written T − skI in place of skI − T . This is a strategic move: when deal- ing with characteristic polynomials it is far more convenient to write det(lI − A) to produce a monic polynomial. On the other hand, as you’ll see now, it is better to work on the individual Wk with the nilpotent transformation T j − s I =: N . Wk k k Decomposition of the Stable Eigenspaces (Take 1). Let’s briefly omit subscripts and consider T : W ! W with one eigenvalue s , dim W = d , B a basis for W and [T]B = B.
    [Show full text]